All Tables

Table 1: Experimental OII Stark widths $W_{\rm m}$ ( FWHM), and different calculations: the semi-classical values calculated by Mahmoudi et al. (2004) $W_{\rm MBS}$ , our data obtained with the modified semiempirical approach (Dimitrijevic & Konjevic 1980) $W_{\rm MSE}$ and semi-classical values of Griem (1974) $W_{\rm eG}$ . References: a. Platisa et al. (1975); b. del Val et al. (1999); c. Djenize et al. (1998); d. Blagojevic et al. (1999); e. Djenize et al. (1991), with e $^{\ast }$ is denoted the line where only the shift is reported by Djenize et al. (1991) and f. Sreckovic et al. (2001). The data indicated by $\dag$ are calculated here and not in the cited paper. The $W_{\rm eG}$ data for T=60000 K denoted by $\top$ are extrapolated Griem (1974) values from Djenize et al. (1991).
Table 2: Calculated OII widths for the transition array $\rm 2p^{2}(^3P)3s -2p^{2}(^3P)3p$ : semi-classical (Griem 1974) values $W_{\rm D}$ calculated by Dimitrijevic (1982), semi-classical (Sahal-Bréchot 1969a,b) values $W_{\rm MBS}$ calculated by Mahmoudi, Ben Nessib and Sahal-Bréchot (2004) and our calculation with the modified semiempirical approach (Dimitrijevic & Konjevic 1980) $W_{\rm MSE}$ . $\lambda _{\rm m}$ is the average wavelength for the multiplet.